Compressible turbulence in the planetary magnetosheaths and the solar wind: spectral properties and estimation of the turbulent cascade rate
Lina Hadid1, Nahuel Andrés2, Fouad Sahraoui3, Sébastien Galtier3, Shiyong Huang4, Norberto Romanelli5,6, Vincent David7, Gina A DiBraccio8, Jasper S Halekas9 and Pablo Dmitruk10, (1)Laboratory of Plasma Physics, École Polytechnique, CNRS, Palaiseau, France, (2)Physics Department, University of Buenos Aires (UBA), Buenos Aires, Argentina, (3)Laboratoire de Physique des Plasmas, Palaiseau, France, (4)Wuhan University, Wuhan, China, (5)LATMOS, Université Pierre et Marie Curie, Paris, France, (6)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (7)Laboratoire de Physique des Plasmas, Saint-Maur Des Fossés Cedex, France, (8)University of Michigan, Ann Arbor, United States, (9)University of Iowa, Department of Physics and Astronomy, Iowa City, IA, United States, (10)Consejo Nacional de Investigaciones Científicas y Técnicas - Phys. Dept. UBA, Departamento de Física - UBA, Buenos Aires, Argentina
